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Night Sky Checklist October–November
Night Sky Checklist October–November

... period of about 5.4 days. Although it is fairly faint even at its best at magnitude 3.6, there are some similar brightness stars near it that help observers notice when its brightness drops off. Algol is an eclipsing variable star in Perseus. Only moderately bright at best at magnitude 2.1, it dims ...
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... • Very long ago planets would not contain enough heavy elements. • We need to have elements past the first generation star level for living things. (need supernova for fusion of elements heavier than iron) ...
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... 360° in 25,772 years. [Note: Each degree contains 360°, and each degree contains 3600 arc seconds.] Because the Earth tilts on its axis at 23½° and slowly wobbles, while it is rotating and orbiting around the Sun, a line drawn through both poles will trace out a cone in the sky above each pole. Henc ...
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... distance, they get extreme near the hole. You are stretched because your feet are nearer than your head, and you are compressed because your shoulders are converging on the singularity. An outside observer sees you getting dimmer and redder, and your watch looks like it runs more slowly. Finally you ...
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... Auriga is located north of the celestial equator. Its name is the Latin word for "charioteer", associating it with various mythological charioteers, including Erichthonius and Myrtilus. Auriga is most prominent in the northern Hemisphere winter sky, along with the five other constellations that have ...
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... The largest known asteroid in the solar system is Ceres, which is located in an orbit between Mars and Jupiter. Although the existence of Ceres has been known for two hundred years, its mass is still not well determined. Suppose the magnitude of the gravitational force between the sun and Ceres equa ...
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R136a1



RMC 136a1 (usually abbreviated to R136a1) is a Wolf-Rayet star located at the center of R136, the central condensation of stars of the large NGC 2070 open cluster in the Tarantula Nebula. It lies at a distance of about 50 kiloparsecs (163,000 light-years) in the Large Magellanic Cloud. It has the highest mass and luminosity of any known star, at 265 M☉ and 8.7 million L☉, and also one of the hottest at over 50,000 K.
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